Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Valley-Inverted Channel Transition in Arabia Terra:   ESP_067636_1875   ESP_067504_1875   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.578

26.2

-1.2

15.33

42.0

41.2

Gullied Slope:   ESP_067695_1430   ESP_068104_1430   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.7

222.

-7.1

23.60

48.2

52.8

Layered Terrain:   ESP_067570_1815   ESP_067702_1815   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.565

26.8

8.49

-8.15

39.7

41.0

Planum Australe:   ESP_067626_0960   ESP_067613_0960   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-83.8

330.

2.80

-4.09

78.7

79.0

Hydaspis Chaos:   ESP_067374_1825   ESP_074852_1825   (Interval in Earth days: 582)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.223

335.

-5.0

-17.0

41.3

52.8

Maja Valles:   ESP_067309_1980   ESP_067441_1980   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.70

305.

7.40

-10.2

48.1

48.1

Terrain Sample Northwest of Sytinskaya Crater:   ESP_067520_2235   ESP_068061_2235   (Interval in Earth days: 42)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.15

305.

4.04

14.32

62.6

55.5

Terrain in Utopia Planitia:   ESP_067356_2140   ESP_067633_2140   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.51

102.

-6.9

15.82

58.5

53.9

Candidate ExoMars Landing Site in Oxia Planum:   ESP_067519_1980   ESP_076830_1980   (Interval in Earth days: 725)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.84

336.

8.05

-2.37

46.3

40.9

Reull Vallis:   ESP_067317_1405   ESP_067726_1405   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

96.4

-6.7

3.611

44.5

49.4


  


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